在GRAPE-6上对天王星-海王星区域内的星子进行29.5 Tflops模拟

J. Makino, E. Kokubo, T. Fukushige, H. Daisaka
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引用次数: 14

摘要

作为2002年戈登贝尔性能奖的参赛作品,我们报告了用于模拟天王星-海王星区域原行星-小行星系统早期演化的GRAPE-6系统的性能。GRAPE-6是用于天体物理n体计算的专用计算机。目前的配置有2048个定制流水线芯片,每个芯片包含6个流水线处理器,用于计算粒子之间的引力相互作用。其理论峰值性能为63.4 Tflops。实际获得的性能为29.5 Tflops,用于模拟具有180万个星子和两个大质量原行星的外太阳系的早期演化。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
A 29.5 Tflops Simulation of Planetesimals in Uranus-Neptune Region on GRAPE-6
As an entry for the 2002 Gordon Bell performance prize, we report the performance achieved on the GRAPE-6 system for a simulation of the early evolution of the protoplanet-planetesimal system of the Uranus-Neptune region. GRAPE-6 is a special-purpose computer for astrophysical N-body calculations. The present configuration has 2048 custom pipeline chips, each containing six pipeline processors for the calculation of gravitational interactions between particles. Its theoretical peak performance is 63.4 Tflops. The actual performance obtained was 29.5 Tflops, for a simulation of the early evolution of outer Solar system with 1.8 million planetesimals and two massive protoplanets.
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